Wils_SDSSJ091741.29+073647.4 = TCPJ09174122+0736487: new SU UMa-type dwarf nova
Itoh-san reported observations on four nights and detected
developing superhumps since Jan. 13. The superhump period is
0.06462(8) d (stage A or A+B combined). The current amplitude
is 0.2 mag.
Gaia18bvd = ASASSN-24ab: new SU UMa-type dwarf nova
Josch Hambsch has reported observations on two nights.
Superhumps with a period of 0.06363(7) d and an amplitude
of 0.20 mag were clearly detected.
Gaia24aaq: new SU UMa-type dwarf nova
Berto Monard reported observations on four nights.
Superhumps were present on three nights. The period
is 0.05527(2) d and the amplitude is 0.21 mag.
ATLAS23xus = TCPJ03433597-1153124: ordinary superhumps
The most recent data (Jan. 2) by Itoh-san recorded probable
ordinary superhumps (rather fragmentary data).
The long waiting time and the large outburst amplitude
suggest a WZ Sge star.
TCP J04251906+2841462: ordinary superhumps
According to Itoh-san's observations, this object showed
ordinary superhumps since Dec. 3. The current period
is 0.05510(4) d. The large amplitude (0.18 mag) seems
to preclude a very low-q object.
TCP J02011347+0139431: new WZ Sge-type dwarf nova
Itoh-san and Kiyota-san detected early superhumps on
two consecutive nights.
Typical double-wave modulations with a period of 0.05746(5) d
(full amplitude 0.06 mag).
TCP J18414194+2153095: new SU UMa-type dwarf nova
Itoh-san detected superhumps on two nights (Nov. 28 and
Dec. 3). The period has not been determined due to this large
gap.